Sodium-22, Al-26, and Be-10 in He-3-rich flares

Details Sodium-22, Al-26, and Be-10 in He-3-rich flares Sodium-22, Al-26, and Be-10 in He-3-rich flares

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979metic..14...43h&link_type=abstract

Meteoritics, vol. 14, Mar. 31, 1979, p. 43-50.

Computer Science

Abundance, Helium Isotopes, Metals, Solar Cosmic Rays, Solar Flares, Aluminum 26, Beryllium 10, Sodium 22, Boron, Sodium, Helium, Oxygen, Abundance, Neon, Magnesium, Carbon, Hydrogen, Isotopes, Flares, Beryllium, Reduction, Allende Meteorite, Meteorites, Aluminum, Isotopic Ratios, Composition, Solar Cosmic Rays, Radioactivity

Scientific paper

The theory of He-3-rich flares by Colgate et al. (1977) implies that the composition of the solar cosmic ray-event associated with a He-3-rich flare is grossly nonsolar. The relative abundances (relative to hydrogen) of carbon, nitrogen, and oxygen, as well as those of heavier elements are significantly reduced, and the isotopic compositions of virtually all elements are bound to be strongly anomalous. In addition, the abundances of Na-22, Al-26, and Be-10 (of which there are approximately 10 to the 25th power atoms each in a He-3-rich flare) are at least comparable to the abundances of stable isotopes of these elements. Conditions for the detectability of the three radioactive species are discussed.

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